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Landed Planetary Sensor Model Support with the Community Sensor Model 利用社区传感器模型支持着陆行星传感器模型
Research notes of the AAS Pub Date : 2024-09-17 DOI: 10.3847/2515-5172/ad7b2e
Jason R. Laura, Oleg Alexandrov and Adam Paquette
{"title":"Landed Planetary Sensor Model Support with the Community Sensor Model","authors":"Jason R. Laura, Oleg Alexandrov and Adam Paquette","doi":"10.3847/2515-5172/ad7b2e","DOIUrl":"https://doi.org/10.3847/2515-5172/ad7b2e","url":null,"abstract":"This note describes recent work to develop landed planetary sensor model support conforming to the widely adopted Community Sensor Model (CSM) standard. We describe the CSM specification and its use in the planetary sciences, introduce the test sensors carried aboard the Mars Science Laboratory Curiosity Rover, and describe the engineering research requirements fulfilled. Ultimately, we demonstrate use of a CSM framing sensor model for the NavCam and MastCam instruments including stereo terrain extraction and map projection using the NASA Ames Stereo Pipeline over a multi-day traverse and multi-image correspondence identification needed as an input to stereophotogrammetric block bundle adjustment using the USGS-maintained Integrated Software for Imagers and Spectrometers library.","PeriodicalId":74684,"journal":{"name":"Research notes of the AAS","volume":"47 1","pages":""},"PeriodicalIF":0.0,"publicationDate":"2024-09-17","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142250313","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
New Pulsating Variable Stars and Eclipsing Binaries Around BL Cam* BL凸轮*周围的新脉冲变星和食双星
Research notes of the AAS Pub Date : 2024-09-16 DOI: 10.3847/2515-5172/ad7b2b
Ai-Ying Zhou
{"title":"New Pulsating Variable Stars and Eclipsing Binaries Around BL Cam*","authors":"Ai-Ying Zhou","doi":"10.3847/2515-5172/ad7b2b","DOIUrl":"https://doi.org/10.3847/2515-5172/ad7b2b","url":null,"abstract":"Based on publicly available Transiting Exoplanet Survey Satellite data, I conducted a regional survey around the SX Phe star BL Cam, spanning a radius of two degrees. This research identified 285 new variables including: 96 δ Scuti stars, 56 γ Doradus stars, 17 eclipsing binary systems with three exhibiting pulsating or rotating components, 3 rotating ellipsoidal variable stars, among others. No new SX Phe stars were identified.","PeriodicalId":74684,"journal":{"name":"Research notes of the AAS","volume":"3 1","pages":""},"PeriodicalIF":0.0,"publicationDate":"2024-09-16","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142250315","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
A Strong Lensing Model of RCS1 J0224−0002.5 RCS1 J0224-0002.5 的强透镜模型
Research notes of the AAS Pub Date : 2024-09-15 DOI: 10.3847/2515-5172/ad79f1
Ryan Walker, Keren Sharon, Alexander Navarre, Matthew Bayliss and Michael D. Gladders
{"title":"A Strong Lensing Model of RCS1 J0224−0002.5","authors":"Ryan Walker, Keren Sharon, Alexander Navarre, Matthew Bayliss and Michael D. Gladders","doi":"10.3847/2515-5172/ad79f1","DOIUrl":"https://doi.org/10.3847/2515-5172/ad79f1","url":null,"abstract":"We present the details of a strong lensing model of RCS1 J0224−0002.5, a strong lensing cluster at z = 0.773, based on data from Hubble Space Telescope/WFC3, Advanced Camera for Surveys, and WFC2. Of particular interest in this field is a z = 4.8786 Lyα emitter (LAE), 15″ from the brightest cluster galaxy (BCG) that stretches northwest to west of the BCG in three different images, with a fourth counter-image ∼4″ southeast of the BCG. Using methods consistent with those used in studying five other LAEs in A. Navarre et al., we find that the cluster is best modeled by two cluster-scale dark matter halos aligned nearly perpendicular to each other at the center of the cluster. A z = 2.396 source is also lensed with six images, providing several constraints that were instrumental in producing this model.","PeriodicalId":74684,"journal":{"name":"Research notes of the AAS","volume":"15 1","pages":""},"PeriodicalIF":0.0,"publicationDate":"2024-09-15","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142250314","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
New Transit Timing Observations of WASP-12b from TESS Sectors 71 and 72 从 TESS 第 71 和 72 区段对 WASP-12b 进行的新凌日定时观测
Research notes of the AAS Pub Date : 2024-09-12 DOI: 10.3847/2515-5172/ad7946
Zoutong Shen
{"title":"New Transit Timing Observations of WASP-12b from TESS Sectors 71 and 72","authors":"Zoutong Shen","doi":"10.3847/2515-5172/ad7946","DOIUrl":"https://doi.org/10.3847/2515-5172/ad7946","url":null,"abstract":"I present new transit and occultation timing measurements for the hot Jupiter WASP-12b using data from TESS Sectors 71 and 72, observed in 2023. Using full-phase curve fitting for the first time, I precisely locate both transits and occultations. I report 34 new transit times and sector-specific occultation times, updating the orbital decay rate to −26.310 ± 0.901 ms yr−1. My analysis strongly favors the orbital decay model over constant period and apsidal precession models.","PeriodicalId":74684,"journal":{"name":"Research notes of the AAS","volume":"15 1","pages":""},"PeriodicalIF":0.0,"publicationDate":"2024-09-12","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142217994","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
New Sample of Ultracool Dwarf Benchmarks with Detailed Chemical Characterization 具有详细化学特征的超酷矮星基准新样本
Research notes of the AAS Pub Date : 2024-09-12 DOI: 10.3847/2515-5172/ad79f0
Lucia Fisher, Roman Gerasimov, Evan N. Kirby, Adam J. Burgasser, Chih-Chun Hsu and Lauren M. Weiss
{"title":"New Sample of Ultracool Dwarf Benchmarks with Detailed Chemical Characterization","authors":"Lucia Fisher, Roman Gerasimov, Evan N. Kirby, Adam J. Burgasser, Chih-Chun Hsu and Lauren M. Weiss","doi":"10.3847/2515-5172/ad79f0","DOIUrl":"https://doi.org/10.3847/2515-5172/ad79f0","url":null,"abstract":"Ultracool dwarfs (UCDs) are considered prime targets for galactic archeology due to their abundance, long lifespans, and the sensitivity of their spectra to chemical composition. To calibrate larger surveys, a sample of benchmark UCDs with robust abundances is necessary. We present [Fe/H], [α/Fe] and abundances of 13 elements, inferred from high-resolution spectra of 13 FGK primaries hosting a UCD companion. For a subset of our sample with APOGEE observations, individual abundances agree within 0.06 dex on average.","PeriodicalId":74684,"journal":{"name":"Research notes of the AAS","volume":"3 1","pages":""},"PeriodicalIF":0.0,"publicationDate":"2024-09-12","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142227085","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
Cometary Activity from Minor Planet 2015 VP51 Discovered with Citizen Science 利用公民科学发现小行星 2015 VP51 的彗星活动
Research notes of the AAS Pub Date : 2024-09-10 DOI: 10.3847/2515-5172/ad7854
Maxwell K. Frissell, Colin Orion Chandler, William J. Oldroyd, Chadwick A. Trujillo, Nima Sedaghat, William A. Burris, Jay K. Kueny, Jarod A. DeSpain, Kennedy A. Farrell, Henry H. Hsieh, Mark Jesus Mendoza Magbanua, Scott S. Sheppard, Michele T. Mazzucato, Milton K. D. Bosch, Tiffany Shaw-Diaz, Virgilio Gonano, Al Lamperti, José A. da Silva Campos, Brian L. Goodwin, Ivan A. Terentev and Charles J. A. Dukes
{"title":"Cometary Activity from Minor Planet 2015 VP51 Discovered with Citizen Science","authors":"Maxwell K. Frissell, Colin Orion Chandler, William J. Oldroyd, Chadwick A. Trujillo, Nima Sedaghat, William A. Burris, Jay K. Kueny, Jarod A. DeSpain, Kennedy A. Farrell, Henry H. Hsieh, Mark Jesus Mendoza Magbanua, Scott S. Sheppard, Michele T. Mazzucato, Milton K. D. Bosch, Tiffany Shaw-Diaz, Virgilio Gonano, Al Lamperti, José A. da Silva Campos, Brian L. Goodwin, Ivan A. Terentev and Charles J. A. Dukes","doi":"10.3847/2515-5172/ad7854","DOIUrl":"https://doi.org/10.3847/2515-5172/ad7854","url":null,"abstract":"We report the discovery of cometary activity emanating from minor planet 2015 VP51 outbound from its recent perihelion passage. The activity, in the form of a diffuse tail, was first identified by volunteers of our Citizen Science program Active Asteroids, a NASA Partner program hosted on the Zooniverse platform. This discovery was aided by the recently implemented TailNet artificial intelligence assistant which filters out images with a low likelihood of showing cometary activity. The tail is present in nine images of 2015 VP51 from the Dark Energy Camera and OmegaCAM between UT 2015 August 2 and UT 2015 October 18. We classify 2015 VP51 as a Jupiter-family comet based on its Tisserand parameter with respect to Jupiter TJ = 2.931.","PeriodicalId":74684,"journal":{"name":"Research notes of the AAS","volume":"36 1","pages":""},"PeriodicalIF":0.0,"publicationDate":"2024-09-10","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142217996","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
A Two-month Mini-moon: 2024 PT5 Captured by Earth from September to November 两个月的小月亮：地球在 9 月至 11 月期间捕捉到的 2024 PT5
Research notes of the AAS Pub Date : 2024-09-09 DOI: 10.3847/2515-5172/ad781f
Carlos de la Fuente Marcos and Raúl de la Fuente Marcos
{"title":"A Two-month Mini-moon: 2024 PT5 Captured by Earth from September to November","authors":"Carlos de la Fuente Marcos and Raúl de la Fuente Marcos","doi":"10.3847/2515-5172/ad781f","DOIUrl":"https://doi.org/10.3847/2515-5172/ad781f","url":null,"abstract":"Near-Earth objects (NEOs) that follow horseshoe paths, and approach our planet at close range and low relative velocity, may undergo mini-moon events in which their geocentric energy becomes negative for hours, days or months, but without completing one revolution around Earth while bound. An example of NEO experiencing such a temporarily captured flyby is 2022 NX1, which was a short-lived mini-moon in 1981 and 2022. Here, we show that the recently discovered small body 2024 PT5 follows a horseshoe path and it will become a mini-moon in 2024, from September 29 until November 25.","PeriodicalId":74684,"journal":{"name":"Research notes of the AAS","volume":"34 1","pages":""},"PeriodicalIF":0.0,"publicationDate":"2024-09-09","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142217997","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
Revisiting WASP-19b’s Orbital Evolution: New TESS Data and Apsidal Precession Analysis 重新审视 WASP-19b 的轨道演变：新的 TESS 数据和傲慢潮前序分析
Research notes of the AAS Pub Date : 2024-09-08 DOI: 10.3847/2515-5172/ad77a6
Zoutong Shen
{"title":"Revisiting WASP-19b’s Orbital Evolution: New TESS Data and Apsidal Precession Analysis","authors":"Zoutong Shen","doi":"10.3847/2515-5172/ad77a6","DOIUrl":"https://doi.org/10.3847/2515-5172/ad77a6","url":null,"abstract":"Due to the ongoing debate of whether WASP19b is experiencing orbital decay or apsidal precession, I reexamine the orbital evolution of the hot Jupiter WASP-19b using new TESS data from sectors 09, 36, 62, and 63. My comprehensive analysis of transit and occultation timing variations compares models of constant period, orbital decay, and apsidal precession. Results show no significant preference between orbital decay and apsidal precession models. I find a period change rate of −1.40 ± 0.54 ms yr−1, slower than some previous studies but consistent with others. My apsidal precession analysis yields an eccentricity of 0.00178 and a precession rate of 0.036 deg day−1, differing from recent literature. These findings underscore the complexity of WASP-19b’s orbital dynamics and the need for continued long-term monitoring.","PeriodicalId":74684,"journal":{"name":"Research notes of the AAS","volume":"63 1","pages":""},"PeriodicalIF":0.0,"publicationDate":"2024-09-08","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142227087","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
Determination of the Abundance of Mercury from the Hg ii Line at 5677.10 Å in Late B-type Stars. VI. HD 173524 (46 Dra) 通过 B 型晚期恒星中位于 5677.10 Å 处的 Hg ii 线确定汞的丰度。VI.HD 173524 (46 Dra)
Research notes of the AAS Pub Date : 2024-09-06 DOI: 10.3847/2515-5172/ad76b1
Richard Monier
{"title":"Determination of the Abundance of Mercury from the Hg ii Line at 5677.10 Å in Late B-type Stars. VI. HD 173524 (46 Dra)","authors":"Richard Monier","doi":"10.3847/2515-5172/ad76b1","DOIUrl":"https://doi.org/10.3847/2515-5172/ad76b1","url":null,"abstract":"The weak line of Hg <sc>ii</sc> located at 5677.10 Å is used to measure the mercury abundance in the most massive component of the SB2 HgMn star HD 173524 (46 Dra). This line is detected at 3<italic toggle=\"yes\">σ</italic> above the noise in the adjacent continuum. The synthesis of this line, confirms a large overabundance of mercury, about +5.00 dex, which is less than the excess derived from the 3983.93 Å line in earlier studies. Spectrum synthesis yields estimates of the abundance deficiencies/excesses for sixteen other elements. Helium, carbon, oxygen, magnesium, silicon, chromium and iron are depleted. Phosphorus, titanium, manganese, gallium, strontium, yttrium, zirconium and barium are overabundant. Platinum is very overabundant. For several elements, these new abundances differ from earlier measurements.","PeriodicalId":74684,"journal":{"name":"Research notes of the AAS","volume":"37 1","pages":""},"PeriodicalIF":0.0,"publicationDate":"2024-09-06","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142218000","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
Comment on “Excluding Primordial Black Holes as Dark Matter Based on Solar System Ephemeris” 关于 "根据太阳系星历排除作为暗物质的原始黑洞 "的评论
Research notes of the AAS Pub Date : 2024-09-06 DOI: 10.3847/2515-5172/ad7674
James M. Cline
{"title":"Comment on “Excluding Primordial Black Holes as Dark Matter Based on Solar System Ephemeris”","authors":"James M. Cline","doi":"10.3847/2515-5172/ad7674","DOIUrl":"https://doi.org/10.3847/2515-5172/ad7674","url":null,"abstract":"It was recently claimed (<ext-link ext-link-type=\"arxiv\" xlink:href=\"https://arxiv.org/pdf/2408.10799\" xlink:type=\"simple\">https://arxiv.org/pdf/2408.10799</ext-link>) that solar system ephemeris data can exclude primordial black hole (PBH) dark matter in the mass range 10<sup>18</sup>–10<sup>22</sup> g. I show that this conclusion is based on an implausible, implicit assumption; namely the uncertainty on the solar system mass within 50 au is as small as the uncertainty on the mass of the Sun. Correcting for this error, I find that ephemeris data can only constrain PBH’s with mass below 10<sup>16</sup> g, which is already excluded by constraints on their evaporation via Hawking radiation. Correcting a further error concerning the time-averaged rate of such fluctuations nullifies even this weaker constraint.","PeriodicalId":74684,"journal":{"name":"Research notes of the AAS","volume":"61 1","pages":""},"PeriodicalIF":0.0,"publicationDate":"2024-09-06","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"142227086","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
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